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Traditional large-scale models of reionization usually employ simple deterministic relations between halo mass and luminosity to predict how reionization proceeds. We here examine the impact on modelling reionization of using more detailed models for the ionizing sources as identified within the 100 Mpc/h cosmological hydrodynamic simulation Simba, coupled with post-processed radiative transfer. Comparing with simple (one-to-one) models, the main difference of using Simba sources is the scatterarXiv:2109.03840v1 fatcat:h34ihvj2xjex3jqvfzrz2v6e5m